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Radial velocity information


A plane flying past a radar station: the plane's velocity vector (red) is the sum of the radial velocity (green) and the tangential velocity (blue).

The radial velocity or line-of-sight velocity of a target with respect to an observer is the rate of change of the vector displacement between the two points. It is formulated as the vector projection of the target-observer relative velocity onto the relative direction or line-of-sight (LOS) connecting the two points.

The radial speed or range rate is the temporal rate of the distance or range between the two points. It is a signed scalar quantity, formulated as the scalar projection of the relative velocity vector onto the LOS direction. Equivalently, radial speed equals the norm of the radial velocity, modulo the sign.[a]

In astronomy, the point is usually taken to be the observer on Earth, so the radial velocity then denotes the speed with which the object moves away from the Earth (or approaches it, for a negative radial velocity).
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Radial velocity

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The radial velocity or line-of-sight velocity of a target with respect to an observer is the rate of change of the vector displacement between the two...

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Doppler spectroscopy

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the radial-velocity method, or colloquially, the wobble method) is an indirect method for finding extrasolar planets and brown dwarfs from radial-velocity...

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Velocity

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transverse velocity v R {\displaystyle {\boldsymbol {v}}_{R}} is the radial velocity. The radial speed (or magnitude of the radial velocity) is the dot...

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Methods of detecting exoplanets

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from Earth, i.e. the variations are in the radial velocity of the star with respect to Earth. The radial velocity can be deduced from the displacement in...

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Angular velocity

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the cross-radial velocity as: ω = d ϕ d t = v ⊥ r . {\displaystyle \omega ={\frac {d\phi }{dt}}={\frac {v_{\perp }}{r}}.} Here the cross-radial speed v...

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Stephenson 2 DFK 1

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(19000+6200 −2500 light-years) from comparison with the cluster's radial velocity, considerably closer than the original distance quoted by Stephenson...

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Alpha Centauri

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indicates that a radial velocity analysis might detect a hypothetical planet of 1.8 ME in Alpha Centauri B's habitable zone. Radial velocity measurements...

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High Accuracy Radial Velocity Planet Searcher

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The High Accuracy Radial Velocity Planet Searcher (HARPS) is a high-precision echelle planet-finding spectrograph installed in 2002 on the ESO's 3.6m...

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Minimum mass

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is a widely cited statistic for extrasolar planets detected by the radial velocity method or Doppler spectroscopy, and is determined using the binary...

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Hipparcos

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better calculations of their distance and tangential velocity. When combined with radial velocity measurements from spectroscopy, astrophysicists were...

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Sloan Digital Sky Survey

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Spring 2014. The Multi-object APO Radial Velocity Exoplanet Large-area Survey (MARVELS) monitored the radial velocities of 11,000 bright stars, with the...

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Lists of planets

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Exoplanet Survey Satellite (TESS) mission.   Transit: 4,176 (74.2%)   Radial velocity: 1,090 (19.4%)   Microlensing: 217 (3.9%)   Direct imaging: 78 (1.4%)...

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Antares

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star is circumpolar as the whole continent is above 64° S latitude. Radial velocity variations were observed in the spectrum of Antares in the early 20th...

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Proper motion

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milliarcseconds per year. Knowledge of the proper motion, distance, and radial velocity allows calculations of an object's motion from the Solar System's frame...

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Proxima Centauri

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8±4 days, consistent with a measurement of 92.1+4.2 −3.5 days from radial velocity observations. Because of its low mass, the interior of the star is...

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Luhman 16

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proximity of Luhman 16. The radial velocity of component A is 23.1 ± 1.1 km/s (14.35 ± 0.68 mi/s), and the radial velocity of component B is 19.5 ± 1.2 km/s...

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Arcturus

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companion. In 1993, radial velocity measurements of Aldebaran, Arcturus and Pollux showed that Arcturus exhibited a long-period radial velocity oscillation,...

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Stellar kinematics

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component of stellar motion toward or away from the Sun, known as radial velocity, can be measured from the spectrum shift caused by the Doppler effect...

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Velocity dispersion

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supercluster. By measuring the radial velocities of the group's members through astronomical spectroscopy, the velocity dispersion of that group can be...

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Alphard

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companion white dwarf star. Precise radial velocity measurements have shown variations in the stellar radial velocities and spectral line profiles. The oscillations...

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Peculiar velocity

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position angle and radial velocity. These can be combined through vector addition to state the object's motion relative to the Sun. Velocities for local objects...

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Aldebaran

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way. In 1993 radial velocity measurements of Aldebaran, Arcturus and Pollux showed that Aldebaran exhibited a long-period radial velocity oscillation,...

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Polaris

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showed the three members of the Polaris ternary system. The variable radial velocity of Polaris A was reported by W. W. Campbell in 1899, which suggested...

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List of exoplanets detected by radial velocity

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following is a list of 456 extrasolar planets that were only detected by radial velocity method –– 31 confirmed and 323 candidates, sorted by orbital periods...

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Binary mass function

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orbital period of the binary system, and the peak radial velocity of the observed star. The velocity of one binary component and the orbital period provide...

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40 Eridani

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cause of the radial velocity variations remained inconclusive. Further studies in 2023: 23–24, 44  and 2024 concluded that the radial velocity signal very...

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Coastal ocean dynamics applications radar

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Doppler shift” and allows one to assess the radial velocity of a surface current. That is; the scatter velocity along the line between the hit surface and...

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